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The on-orbit HRMA on-axis effective area predictions are generated from raytracing models and scaled by the HRMA calibration data taken at the XRCF. This is the current best prediction for the HRMA EA, which has already been included in the Chandra Proposers' Observatory Guide.
The CALDB contains the official effective area tables
| Analysis and Presentations | |||
|---|---|---|---|
| Effect of Contamination of the HRMA on the Optics'
Aeff 2005 Chandra User's Committee Presentation |
Diab Jerius (1/25/05) |
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| Effective Area Analysis Using the HETGS: 2005 Chandra User's Committee Presentation | Herman Marshall (1/25/05) |
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| Empirical Corrections to the HRMA Ir M Edge Discrepancy: 2004 Calibration Workshop Presentation | Diab Jerius (10/27/04) |
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| Revisiting Iridium Optical Constants and the Chandra HRMA Effective Area: 2004 Calibration Workshop Presentation | Dale Graessle (10/27/04) |
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| Chandra X-ray Observatory Mirror Effective Area: 2003 Calibration Workshop Presentation | Ping Zhao (10/28/03) |
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| Effective Area of the HRMA Near the Ir M-V Edge at 2.1 keV: 2003 Calibration Workshop Presentation | Herman Marshall (10/28/03) |
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| Chandra X-ray Observatory Mirror Effective Area: 2003 SPIE Paper | Ping Zhao (August 2003) |
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Last modified:12/06/06
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Center (CXC) is operated for NASA by the Smithsonian Astrophysical Observatory. 60 Garden Street, Cambridge, MA 02138 USA. Email: cxcweb@head.cfa.harvard.edu Smithsonian Institution, Copyright © 1998-2004. All rights reserved. |